adaptive optics institute for astronomy david kim
TRANSCRIPT
Adaptive Optics
Institute for Astronomy
David Kim
Introduction
Design Goals
What is Adaptive Optics (AO)
Hardware for AO
Tests and Results
Design Goals
Get Hardware Running
Get Familiar With Hardware
Design A Test Setup
Link Hardware With Software
What Is AO?
Deformable Mirro
r
Shack-Hartmann Wave front Sensor
Wavefront Sensor Data
Wavefront Sensor Data
Wavefront Sensor Data
Vector Display of wave frontVector Components
Boston Micromachines Deformable Mirror
140 Actuators MicroElectroMechanical Systems (MEMS) Continuous or Segmented Deformable Mirror
Interferometer Test of BMC Mirror
Interferometer Test of BMC Mirror
Interferometer Test of BMC Mirror
Test giving left half actuators then right half 100 volts
Interferometers Isometric plots of mirrors surface
Expected to see half of the surface low and the other half high
Interferometer Test of Agile Mirror
Identical Setup just a different mirror
Left half and right half of actuators given 100 volts
Actuator Test of BMC Mirror
Actuator Test of BMC Mirror
Actuator Test of BMC Mirror
Conclusion
Wavefront Sensor Operational
Interferometer Setup Correct
BMC deformable mirror broken
New deformable mirror needed
Thank You Special Thanks JD Armstrong Jeff Kuhn Joe Ritter John Messersmith John Valliant
The Akamai Internship Program is funded by the Center for Adaptive Optics through its National Science Foundation Science and Technlogy Center grant (#AST-987683) and by grants to the Akamai Workforce Initiative from the National Science Foundation and Air Force Office of Scientific Research (both administered by NSF, #AST-0710699) andfrom the University of Hawaii.
Lani Lebron Lisa Hunter Lynne Raschke Mark Hoffman Scott Seagroves